RECON: TNO occultation with 04PX107

Event between 04PX107 and star GA0720:33438758 with event index number of 1188950

Geocentric closest approach at 2022/07/11 04:31:13 UTC

J2000 position of star is 21:41:40.5 -17:00:47
Equinox of date position of star is 21:42:52.6 -16:54:47
Stellar brightness G=16.6, use SENSEUP=128 with the MallinCam and and exposure time of 2 seconds with the QHY174 camera.
Star is 70 degrees from the moon. Moon is 90% illuminated.
TNO apparent brightness V=23.6

TNO is 42.0 AU from the Sun and 41.2 AU from the Earth.
The TNO is moving 19.8 km/sec on the sky relative to the star, or, 2.4 arcsec/hr.
The 1-sigma error in the time of the event is 387 seconds.
The 1-sigma cross-track error in the shadow position is 4505 km.

The TNO has an absolute magnitude Hv=7.3
Diameter=219.8 km assuming a 5% albedo -- 10.8 sec chord
Diameter=89.7 km assuming a 30% albedo -- 4.4 sec chord
Dynamical classification is CLASSICAL
 
 
 
 
 
 
 
 

Star training set for 04PX107, (2022/07/11 04:35UT)
Object            RA         Dec     mag  sep  mel
Fomalhaut      22:58:53.4 -29:30:09  1.2 21.47  82
40Gam Cap      21:41:20.1 -16:33:34  3.7  0.52  70
PPM 239183     21:41:50.8 -16:39:52  8.5  0.35  70
PPM 239227     21:43:32.3 -16:45:58  9.4  0.21  70
04PX107        21:42:54.9 -16:54:35 16.6        70
Positions are for equinox of date

Azimuth is measured in degrees eastward from north. North is at an azimuth of 0, due East is at an azimuth of 90 degrees, due South is 180, and due West is 270.

Do not use the listing below for the RECON CPC 1100 telescopes. This is provided for other non-team facilities.

Star training set for 04PX107, (2022/07/11 04:35UT)
Object            RA         Dec     mag  sep  mel
Fomalhaut      22:57:39.6 -29:37:24  1.2 21.47  82
40Gam Cap      21:40:05.7 -16:39:45  3.7  0.52  70
PPM 239183     21:40:36.4 -16:46:03  8.5  0.35  70
PPM 239227     21:42:18.0 -16:52:11  9.4  0.21  70
04PX107        21:41:40.5 -17:00:47 16.6        70
Positions are for J2000

Event circumstances last updated at 2021/10/26 23:53:46 UT

Marc W. Buie, Southwest Research Institute

RECON